Mwc 342: results and analysis of photometric variations of brightness
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Keywords:
Photometric BVRI, photometric observation, zenith distance, intrinsic polarization, criterion 2 n, brightness variations, periodogram, phase-process diagram.Abstract
The results and analysis of photometric measurements for MWC 342 are given. The photometric BVRI dates were received with CCD camera ST-7 and filters of SBIG. In spite of that R and I filters gives the magnitudes in Johnson-Cousins system, we reduced our observations to the standard Johnson system. All photometric observations were corrected for flat field, received from twilight sky.The cyclic changes of brightness with the period P=5588 of days are found. It is shown that on separate intervals of time the periodic changes with the period 115 days are possible but it is difficult to draw a conclusion about reality of cycle brightness variations on periods 100-200 days.References
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How to Cite
Andreyev, A. V., Kurchakov, A. V., & Rspaev, F. K. (2012). Mwc 342: results and analysis of photometric variations of brightness. International Journal of Mathematics and Physics, 3(1), 40–43. Retrieved from https://ijmph.kaznu.kz/index.php/kaznu/article/view/65
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Chemical Physics and Radio Phisics
